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Astronomy Principles and Practice Fourth Edition.pdf

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Answers to problems<br />

Chapter 7<br />

1. 32 ◦ ,78 ◦ , 259 ◦ ,20 ◦ 55 ′ ,62 ◦ 17 ′ ,28 ◦ 18 ′ , 234 ◦ 09 ′<br />

2. 10 ◦ ,53 ◦ ,17 ◦ 14 ′ , 164 ◦ 41 ′ ,77 ◦ 10 ′<br />

3. 600, 3180, 1034, 9881, 4630<br />

4. 472·1, 3405, 415·7, 1614<br />

5. (i) c = 39 ◦ 59 ′ , B = 48 ◦ 19 ′ , A = 66 ◦ 53 ′<br />

(ii) a = 56 ◦ 22 ′ , B = 70 ◦ 15 ′ , C = 67 ◦ 46 ′<br />

(iii) b = 145 ◦ 29 ′ , A = 69 ◦ 19 ′ , C = 37 ◦ 07 ′<br />

(iv) a = 159 ◦ 00 ′ , A = 44 ◦ 22 ′ , B = 42 ◦ 24 ′<br />

6. (i) 5786 nautical miles (ii) 5220 nautical miles<br />

7. 1 d 19·h77<br />

8. 5582 km; 53 ◦ 48 ′ N<br />

9. 72 ◦ 49 ′<br />

Chapter 8<br />

1. Figures A8.1(a), A8.1(b)<br />

2. Figure A8.2<br />

3. Figure A8.3<br />

4. Figure A8.4<br />

5. λ = 90 ◦ ; β = 21 ◦ 33 ′ N<br />

6. 6 ◦ 34 ′<br />

8. 95 ◦ 55 ′ WofN;95 ◦ 55 ′ EofN<br />

9. 29 ◦ 46 ′ N; 180 ◦ 01 ′ . Dec 21st; June 21st<br />

(Hint: The points of intersection of the galactic equator with the ecliptic must be at <strong>and</strong> )<br />

10. (Hint: PXZ = 90 ◦ when azimuth is a maximum for a circumpolar star)<br />

11. 47 ◦ 42 ′ (3 h 10 m 48 s ); φ ≥ 51 ◦ 16 ′ N<br />

12. 19 ◦ 46 ′<br />

14. 117 ◦ 0·′14 (7 h 48 m 01 s );10 h 57 m 30 s<br />

15. 49 ◦ 57 ′ E<br />

16. 59 ◦ 47 ′ 09 ′′ ;72 ◦ 54 ′ 25 ′′<br />

460

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